(3) A blackbody object emits radiation over a wide range of wavelengths, with a maximum emission per unit wavelength that "peaks" at a particular wavelength that can be calculated with Wien's Displacement Law. If you behave as a blackbody with a temperature of 97\deg F,(a) Calculate the peak wavelength of the radiation you would emit (6 pts).(b) Identify the type of radiation this wavelength corresponds to (e.g., UV, visible light, etc. 4 pts)(c) Calculate the energy you would emit per unit area. (Hint: plug the temperature in Kelvin into the Stefan-Boltzmann Law. 2 pts)